Sensitivity of de-excitation energies of superdeformed secondary minima to the density dependence of symmetry energy with the relativistic mean-field theory

被引:4
作者
Jiang, W. Z. [1 ,4 ]
Ren, Z. Z. [2 ,4 ]
Sheng, Z. Q. [2 ]
Zhu, Z. Y. [3 ,4 ]
机构
[1] Southeast Univ, Dept Phys, Nanjing 211189, Peoples R China
[2] Nanjing Univ, Dept Phys, Nanjing 210093, Peoples R China
[3] Chinese Acad Sci, Inst Appl Phys, Shanghai 201800, Peoples R China
[4] Ctr Theoret Nucl Phys, Natl Lab Heavy Ion Accelerator, Lanzhou 730000, Peoples R China
关键词
ASYMMETRIC NUCLEAR-MATTER; PYGMY DIPOLE RESONANCE; NEUTRON-STAR STRUCTURE; HEAVY-ION REACTIONS; FINITE NUCLEI; ISOSPIN DIFFUSION; EXOTIC NUCLEI; PB-208; RADIUS; EQUATION;
D O I
10.1140/epja/i2010-10962-6
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The relationship between de-excitation energies of superdeformed secondary minima relative to ground states and the density dependence of the symmetry energy is investigated for heavy nuclei using the relativistic mean-field (RMF) model. It is shown that the de-excitation energies of superdeformed secondary minima are sensitive to differences in the symmetry energy that are mimicked by the isoscalar-isovector coupling included in the model. With deliberate investigations on a few Hg isotopes that have data of deexcitation energies, we find that the description for the de-excitation energies can be improved due to the softening of the symmetry energy. Further, we have investigated de-excitation energies of odd-odd heavy nuclei that are nearly independent of pairing correlations, and have discussed the possible extraction of the constraint on the density dependence of the symmetry energy with the measurement of de-excitation energies of these nuclei.
引用
收藏
页码:465 / 471
页数:7
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